Results 101 to 110 of about 726,750 (238)
On the origins of enigmatic stellar populations in Local Group galactic nuclei [PDF]
We consider the origins of enigmatic stellar populations in four Local Group galactic nuclei, specifically the Milky Way, M31, M32 and M33. These are centrally concentrated blue stars, found in three out of the four nuclear star clusters (NSCs ...
N. Leigh +4 more
semanticscholar +1 more source
We present a novel pair of numerical models of the interaction history between the Large and Small Magellanic Clouds (LMC and SMC, respectively) and our Milky Way (MW) in light of recent high precision proper motions (Kallivayalil et al. 2006a,b).
Agertz +161 more
core +1 more source
The Impact of Stellar Collisions in the Galactic Center
We consider whether stellar collisions can explain the observed depletion of red giants in the Galactic center. We model the stellar population with two different IMFs: 1) the Miller-Scalo and 2) a much flatter IMF. In the former case, low-mass main-sequence stars dominate the population, and collisions are unable to remove red giants out to 0.4 pc ...
Davies, M. B. +5 more
openaire +2 more sources
The LMC’s stellar bar is offset from the outer disk center, tilted from the disk plane, and does not drive gas inflows. These properties are atypical of bars in gas-rich galaxies, yet the LMC bar’s strength and radius are similar to typical barred ...
Himansh Rathore +3 more
doaj +1 more source
The Birth of High Mass Stars: Accretion and/or Mergers?
The observational consequences of the merger scenario for massive star formation are explored and contrasted with the gradual accumulation of mass by accretion.
Bernasconi P. A. +25 more
core +1 more source
Globular Cluster Formation from Colliding Substructure
We investigate a scenario where the formation of Globular Clusters (GCs) is triggered by high-speed collisions between infalling atomic-cooling subhalos during the assembly of the main galaxy host, a special dynamical mode of star formation that operates
Burkert, Andreas +4 more
core +1 more source
Gravitationally Induced Explosive Outflows
Over the past decade, there has been a significant increase in the reporting of extensive and luminous star-forming regions associated with explosive outflows.
P. R. Rivera-Ortiz +6 more
doaj +1 more source
Recent progress in a quantitative study of the 12C+12C sub-Coulomb fusion is reported. It is carried out using full-dimensional, time-dependent wave-packet dynamics, a quantum reaction model that has not been much exploited in nuclear physics, unlike in ...
Diaz-Torres Alexis, Wiescher Michael
doaj +1 more source
Mg line formation in late-type stellar atmospheres: II. Calculations in a grid of 1D models [PDF]
Mg is the alpha element of choice for Galactic population and chemical evolution studies as it is easily detectable in all late-type stars. Such studies require precise elemental abundances, and thus departures from LTE need to be accounted for. Our goal
Y. Osorio, P. Barklem
semanticscholar +1 more source
Quasi-Periodic Flares from Star-Accretion Disc Collisions
We present simulated results of quasi-periodic flares generated by the inelastic collisions of a star bound to a super-massive black hole (SMBH) and its attendant accretion disc.
Alexander +67 more
core +1 more source

